Just over two weeks after its dark silhouette crossed in front of the Sun for
parts of the Pacific and the Americas, it is the Moon's turn to undergo an eclipse.
Early on Sunday morning, April 24, the Moon will quietly slip into the Earth's
outer shadow, known as the penumbra. While a penumbral eclipse is less dramatic
than partial or total eclipses, avid skywatchers will be setting their alarm
clocks early.
North and South America are in the best position to see this event.
In a penumbral eclipse, no part of the Moon enters the dark umbral shadow of
the Earth, so no part of the Moon shows the distinct outline of the Earth's
shadow. Since it will pass through the outer extremities of the Earth's shadow,
this is a pale eclipse that will do little to moderate the Moon's light. That
part of the Moon closest to the much darker shadow of the Earth (called the
umbra) may exhibit a sensible darkening, but it might not catch the eye.
The penumbral shadow is usually faint and difficult to perceive unless at least
two-thirds of the Moon's disk is immersed within it. Also, one edge of the Moon
should closely approach the much darker umbral shadow.
If seen from the Moon, the Earth would appear to partly eclipse the Sun.
In order to see it, Americans will have be up during the wee hours of the morning,
as our timetable
indicates. The best views will be for Alaska, Hawaii and western North America
where the Moon will be high in the sky. Farther east, the Moon will appear lower
in the sky and for the eastern U.S. and Canada, morning twilight will be in
progress as the Full Moon descends the western sky.
The timetable
provides the moment when the Moon will start to enter the penumbral shadow,
but absolutely nothing unusual will be noticed on the lunar disk at that time.
At the time of the darkest phase of the eclipse, the eclipse magnitude - that
is, the percentage of the Moon's diameter that is within the lighter penumbral
shadow - will equal 89.0 percent.
The Moon will be passing through the southern part of the Earth's penumbra
and its uppermost edge will miss touching the umbra by about only about 237
miles. Perhaps for about 25 minutes before and after this time, that uppermost
portion of the Moon should appear lightly "smudged" or shaded, especially
through binoculars and low-power telescopes.
The eclipse will also be visible from eastern Asia, Indonesia, Australia and
New Zealand, however for these regions, the eclipse is a Sunday evening event;
the Moon will already be within the penumbra as it rises, except for eastern
Australia and New Zealand where the eclipse starts after moonrise. For the rest
of the world, this event will happen during the daylight hours with the Moon
below the horizon, hence the eclipse will not be visible.
If that is case for you, don't fret too much. This is, after all a rather underwhelming
event.
Timetable for the April 24, 2005 penumbral lunar eclipse
| |
EDT
|
CDT
|
MDT
|
PDT
|
|
Moon Enters Penumbra
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3:50 a.m.
|
2:50 a.m.
|
1:50 a.m.
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12:50 a.m.
|
|
Faint smudge appears?
|
5:30 a.m.
|
4:30 a.m.
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3:30 a.m.
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2:30 a.m.
|
|
Maximum ("darkest") eclipse
|
5:55 a.m.
|
4:55 a.m.
|
3:55 a.m.
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2:55 a.m.
|
|
Faint smudge disappears?
|
6:20 a.m.
|
5:20 a.m.
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4:20 a.m.
|
5:20 a.m.
|
|
Moon Leaves Penumbra
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After Moon sets
|
After Moon sets
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6:00 a.m.
|
5:00 a.m.
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Joe Rao
serves as an instructor and guest lecturer at New York's Hayden Planetarium.
He writes about astronomy for The New York Times and other publications, and
he is also an on-camera meteorologist for News
12 Westchester, New York.